Jupiter
Contents
Quick Facts
Mythology
Core
Outermost Layer
Cloud Layers
Winds
Rings
Bringer of Jollity
 
 
Quick Facts:
Jupiter is the fifth planet from the Sun and by far the largest.
Jupiter is more than twice as massive as all the other planets combined (318 times Earth).
Jupiter is about 90% hydrogen and 10% helium with traces of methane, water, ammonia and rock.
Jupiter's Great Red Spot is a hurricane.
Distance from the Sun: 778,330,000 km (483,400,000 miles or 5.20 AU)
Period of Revolution: 11.86 years
Diameter: 142,984 km (88,700 miles)
Mass: 1.900e27 kg
Satellites: 16- Metis, Adrastea, Amalthea, Thebe, Io, Europa, Ganymede, Callisto, Leda, Himalia, Lysithea, Elara, Ananke, Carme, Pasiphae, and Sinope.

Mythology:
Jupiter was the King of the Gods, the ruler of Olympus and the patron of the Roman state. Zeus was the son of Cronus (Saturn).
 
Core:
Above the core lies the main bulk of the planet in the form of liquid metallic hydrogen. This exotic form of the most common of elements is possible only at pressures exceeding 4 million bars, as is the case in the interior of Jupiter. Liquid metallic hydrogen consists of ionized protons and electrons. At the temperature and pressure of Jupiter's interior hydrogen is a liquid, not a gas. It is an electrical
conductor and the source of Jupiter's magnetic field. This layer probably also contains some helium and traces of various ices.

Outermost Layer:
The outermost layer is composed primarily of ordinary molecular hydrogen and helium which is liquid in the interior and gaseous further out. The atmosphere we see is just the very top of this deep layer. Water, carbon dioxide, methane and other simple molecules are also present in tiny amounts.

Cloud Layers:
Three distinct layers of clouds are believed to exist consisting of ammonia ice, ammonium hydrosulfide and a mixture of ice and water. The vivid colors seen in Jupiter's clouds are probably the result of subtle chemical reactions of the trace elements in Jupiter's atmosphere, perhaps involving sulfur whose compounds take on a wide variety of colors, but the details are unknown. The colors correlate with the cloud's altitude: blue lowest, followed by browns and whites, with reds highest. Sometimes we see the lower layers through holes in the upper ones.

Winds:
Jupiter and the other gas planets have high velocity winds which are confined in wide bands of latitude. The winds blow in opposite directions in adjacent bands. Slight chemical and temperature differences between these bands are responsible for the colored bands that dominate the planet's appearance. The light colored bands are called zones, the dark ones belts. The data from the Galileo probe indicate that the winds are even faster than expected (more than 400 mph) and extend down into as far as the probe was able to observe. Jupiter's atmosphere was also found to be quite turbulent. This indicates that Jupiter's winds are driven in large part by its internal heat rather than from solar input as on Earth.

Rings:
Jupiter has faint rings like Saturn's, but much smaller. They were totally unexpected and were only discovered when two of the Voyager 1 scientists insisted that after traveling 1 billion km it was at least worth a quick look to see if any rings might be present. They have since been imaged in the infra-red from ground based telescopes.